轻型航空发动机二级涡轮增压匹配模拟

为了使现有轻型航空发动机在海拔高度为10km的高空保持原有动力性不变,需要采用二级涡轮增压,保持发动机在不同海拔高度时稳压腔内的进气密度与海平面的一致.对原发动机在一级涡轮增压的基础上进行二级涡轮增压匹配.这里采用AVL-Boost软件建模,根据实验校验一级涡轮增压模型,然后建立二级涡轮增压模型.考虑小型离心式压气机高...     

涡流阀几何参数对固体发动机推力调节特性的影响

为了获得涡流阀参数对发动机推力调节性能的影响规律,针对涡流阀的加注方式以及几何结构,利用建立的基于涡流阀方案的固体火箭发动机推力可调实验系统开展了实验研究。通过实验结果的分析,得到了加注环孔径、涡流室高度和直径以及中心进气面积的不同对涡流阀调节性能的影响规律。结果表明:适当降低涡流室的高度、较大的中心进气面积、较大的涡流室直径有利于提高涡流阀的调节性能。因此,可以通过对涡流阀结构的优化设计来提高发动机的推力调节性能。     

某涡扇发动机考虑级间引气的二维数值模拟

针对采用S₂流面流场模拟软件(AES-S2),对某涡扇发动机风扇、压气机(考虑级间引气)和整机进行地面0km及高空21km低雷诺数工况下转速特性的评估和流场分析.AES-S2数值仿真模型由带有黏性项的二维欧拉方程、燃烧模型和损失模型构成;采用任意曲线坐标系,可保证复杂几何边界的计算精度;采用隐式高阶精度Godunov求解格式,数值稳定性高,可自动捕捉激波.仿真结果表明:AES-S2计算稳定性好,收敛速度快;风扇和压气机的计算精度高于整机;整机二维计算满足工程精度需求,可为部件研制和整机部件匹配提供性能参数依据.      

基于光谱分析技术的磨损故障监测

采用转盘电极式原子发射光谱分析技术,监测某型燃气轮机传动润滑系统磨损状况的发展变化趋势,及时诊断早期磨损故障.为确保光谱分析技术监测的准确性,着重研究了环境温度波动、标准曲线细化、样品黏度以及磨损颗粒尺寸等主要因素对测量结果的影响,并简要阐述了光谱分析技术的基本原理.经大量研究试验表明:光谱分析技术能够提前预报燃气轮机传动润滑系统可能发生的磨损故障,是油液状态监控的1种有效手段.     

涡扇发动机极值限制保护闭环控制设计

现代高性能涡扇发动机采用分段组合多变量控制计划,以发挥发动机工作在整个飞行包线范围内的气动热力设计潜力。为保证发动机在过渡态工作的安全性,控制系统中必须考虑极值限制保护控制的设计问题。为避免直接限制保护控制引发的不同控制通道切换带来的系统震荡问题,提出1种高回路稳态增益的滞后-超前频域校正间接极值限制保护控制器设计方法,在保证限制回路足够的稳态精度和抗噪声能力的同时,又避免了引入积分环节导致相角裕度损失过大的缺点。通过发动机线性模型和非线性模型的控制系统仿真,验证了所述方法设计限制控制器的有效性。     

基于状态维修策略下的数据自动获取技术

阐述了在基于状态的维修策略下飞机状态参数的自动获取技术的实现过程和此过程中的技术难点,突破了飞机原厂家默认触发的状态数据的局限性,验证了以自主状态报文获取所需飞机状态数据的技术可行性,实现了飞机状态数据的自主筛选与传递。     

Lateral Flight Technical Error Estimation Model for Performance Based Navigation

Flight technical error (FTE) combined with navigation system error (NSE) is the main part of total system error (TSE) in performance based navigation (PBN).The implementation of PBN requires pre-flight prediction and en-route short-term dynamical prediction of the TSE.Once the sum of predicted lateral FTE and NSE is greater than the specified PBN value,the PBN cannot operate.Thus,accurate modeling and thorough analysis of lateral FTE are indispensible.Multiple-input multiple-output (MIMO) lateral track control system of a transport aircraft is designed using linear quadratic Gaussian and loop transfer recovery (LQG/LTR) method,and the lateral FTE of a turbulence disturbed approach operation is analyzed.The error estimation mapping function of latera FTE and its bound estimation algorithm are proposed based on singular value theory.According to the forming mechanism of lateral FTE,the algorithm considers environmental turbulence fluctuation disturbance,aircraft dynamics and control system parameters.Real-data-based Monte-Carlo simulation validates the theoretical analysis of FTE.It also shows that FTE is mainly caused by turbulence fluctuation disturbance when automatic flight control system (AFCS) is engaged and would increase with escalating environmental turbulence intensity.     

造型细节和离地间隙对轿车气动性能影响研究_修改稿

汽车造型的不同处理方法、发动机安放位置、离地间隙、发动机舱冷却风的排出模式对轿车气动性能产生影响。应用FLUENT软件，分别对汽车造型的不同处理方法、发动机安放位置、离地间隙、发动机舱冷却风的排出模式进行气动性能仿真。结果表明：汽车造型的处理方法中以加车轮和加发动机舱对气动性能影响最大，发动机存在最佳的安放位置，不同的离地间隙对仿真结果影响很大，选择发动机舱冷却风的排出模式要综合考虑阻力系数和升力系数。     

Occurrence rate of SAR arcs during the 23rd solar activity cycle

The occurrence rate of SAR arcs during 1997–2007 has been analyzed based on the photometric observations at the Yakutsk meridian (Maimaga station, corrected geomagnetic coordinates: 57°N, 200°E). SAR arcs appeared in 114 cases (∼500 h) during ∼370 nights of observations (∼3170 h). The occurrence frequency of SAR arcs increases to 27% during the growth phase of solar activity and has a clearly defined maximum at a decline of cycle 23. The SAR arc registration probability corresponds to the variations in geomagnetic activity in this solar cycle. The dates, intervals of UT, and geomagnetic latitudes of SAR arc observations at the Yakutsk meridian are presented.     

Probing solar and stellar interior dynamics and dynamo

Solar and stellar activity is a result of complex interaction between magnetic field, turbulent convection and differential rotation in a star’s interior. Magnetic field is believed to be generated by a dynamo process in the convection zone. It emerges on the surface forming sunspots and starspots. Localization of the magnetic spots and their evolution with the activity cycle is determined by large-scale interior flows. Thus, the internal dynamics of the Sun and other stars hold the key to understanding the dynamo mechanism and activity cycles. Recently, significant progress has been made for modeling magnetohydrodynamics of the stellar interiors and probing the internal rotation and large-scale dynamics of the Sun by helioseismology. Also, asteroseismology is beginning to probe interiors of distant stars. I review key achievements and challenges in our quest to understand the basic mechanisms of solar and stellar activity.